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## DIRECTIONS FOR RUNNING THE ARPS MODEL FOR THE 30-M TORNADO SIMULATION PRESENTED IN OLIVERA ET AL. 2022 ##
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 THE ARPS NAMELIST FILES HEREIN CORRESPOND ARE USED TO RUN ARPS v. 5.4 AT 30-M HORIZONTAL GRID SPACING TO PRODUCE
 AN IDEALIZED (HORIZONTALLY HOMOGENEOUS) SIMULATION OF A VIOLENT TORNADO. THE SIMULATION USES A GRIDPOINT PROFILE 
 EXTRACTED FROM A REAL-DATA WRF SIMULATION OF THE 27 APRIL 2011 TORNADO OUTBREAK IN THE SE U.S. 40 KM UPSTREAM
 OF THE MODEL-EQUIVALENT FOR TUSCALOOSA TORNADIC SUPERCELL AT 2100 UTC. THE SIMULATION WAS RUN ON STAMPEDE2 
 (TACC/UTEXAS, VIA XSEDE).

 THERE ARE 19 NAMELIST FILES, EACH FOR A 600-S INTERVAL OF THE TOTAL 10800 S OF SIMULATION TIME. THUS, THE SIMULATION 
 IS AT 0-600 S, 600-1200 S, ETC. DUE TO TECHNICAL ISSUES ON STAMPEDE2 AT THE TIME, THE SIMULATION WAS STOPPED DURING
 THE 7200-7500 S MODEL TIME. THE SIMULATION WAS THEN RESTATED AT 7500 S AND PROCEEDED AT THE REGULAR 600-S INTERVALS
 UNTIL 10500 S AND FINISHED AT 10500 S FOLOWING A 300-S RUN (I.T., IT WAS RUN AT 7500-8100 S, ... 9900-10500 S 
 INTERVALS AND THEN 10500-10800 S).

 TO RUN THE SIMULATION ON STAMPEDE2 (EXAMPLE):
 ibrun arps_mpi_compiled_code /input_directory/arps_30m_27April2011_Tuscaloosa_supercell_t0-600s.input >& /output_directory/arps_30m_27April2011_Tuscaloosa_supercell_t0-600s.output

 FOR MORE INFORMATION ON THE SIMULATION SPECIFICS, PLEASE CONSULT OLIVEIRA ET AL. (2022) OR CONTACT DR. MING XUE 
 (MXUE@OU.EDU), DR. MAURICIO I. OLIVEIRA (MAURICIO.OLIVEIRA-1@OU.EDU OR MAURICIO.METEOROLOGIA@GMAIL.COM).

